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researcher

M. Lilley

8 papers hereh-index 7300 citations12 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author1
  • first author1
  • middle author4
  • last author2

Across the 8 of 8 papers where every author was matched, so the position is known.

fields
  • astro-ph5
  • hep-ph3
same name
  • M. Lilley — 19 papers, h 21
  • M. Lilley — 5 papers, h 5
  • M. Lilley — 3 papers, h 10
  • M. Lilley — 3 papers, h 2
  • M. Lilley — 1 paper
  • M. Lilley — 1 paper, h 2

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
19992001
most citedQuintessence and the Separation of CMB Peaks

127 citations · 369 across the 8 of their papers we have counts for

collaborators
Showing 2001Show all

4 papers · 1 filter

astro-ph2001★ 7 cited

The Influence of Quintessence on the Separation of CMB Peaks

Michael Doran, Matthew Lilley, Jan Schwindt +1

A hypothetical dark energy component may have an equation of state that is different from a cosmological constant and possibly even changing in time. The spacing of the cosmic micr…

astro-ph2001★ 30 cited

Constraining Quintessence with the New CMB Data

Michael Doran, Matthew Lilley, Christof Wetterich

The CMB data recently released by BOOMERANG and MAXIMA suggest that the anisotropy spectrum has a third peak in the range 800<l_3<900. A combination of this result with constraints…

astro-ph2001★ 77 cited

The Location of CMB Peaks in a Universe with Dark Energy

Michael Doran, Matthew Lilley

The locations of the peaks of the CMB spectrum are sensitive indicators of cosmological parameters, yet there is no known analytic formula which accurately describes their dependen…

hep-ph2001★ 5 cited

Defect Formation Rates in Cosmological First-Order Phase Transitions

Matthew Lilley, Antonio Ferrera

In cosmological first-order phase transitions, the progress of true-vacuum bubbles is expected to be significantly retarded by the interaction between the bubble wall and the hot p…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.